Constraints on Large-Scale Magnetic Fields from the Auger Results

Simple item page
dc.creatorDe Angelis, Alessandro
dc.creatorPersic, Massimo
dc.creatorRoncadelli, Marco
dc.date2007-11-21
dc.date2008-02-25
dc.date.accessioned2026-07-07T11:13:19Z
dc.date.available2026-07-07T11:13:19Z
dc.descriptionA recent article from the Pierre Auger Collaboration links the direction of charged cosmic rays to possible extragalactic sites of emission. The correlation of the direction of such particles with the direction of the emitter allows constraining the value of large-scale magnetic fields B. Assuming for B a coherence length in the range between 1 Mpc and 10 Mpc, we find values of B between 0.3 and 0.9 nG.
dc.description3 pages, no figures
dc.identifierhttps://arxiv.org/abs/0711.3346
dc.identifierhttp://arxiv.org/abs/0711.3346
dc.identifierMod.Phys.Lett.A23:315-317,2008
dc.identifierdoi:10.1142/S0217732308026431
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/191677
dc.subjectAstrophysics
dc.titleConstraints on Large-Scale Magnetic Fields from the Auger Results
dc.typetext

Files

Collections

arXiv